A statistical study of Cluster and ground-based observations of Pi1B pulsations at substorm onset

Physics

Scientific paper

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[2431] Ionosphere / Ionosphere/Magnetosphere Interactions, [2487] Ionosphere / Wave Propagation, [2752] Magnetospheric Physics / Mhd Waves And Instabilities, [2790] Magnetospheric Physics / Substorms

Scientific paper

Recent studies have shown that Pi1B pulsations, observed on the ground at substorm onset, are not a result of small-scale ionospheric currents but have their origins within the magnetosphere. In addition, various case studies have shown that corresponding Pi1B signatures in space are, in fact, Doppler shifted observations of the magnetic signature of fast flows. In order to explore the relationship between ground- and space-based observations further, we have carried out a statistical study of 300 Pi1B events observed by the Cluster spacecraft during 2001-2004, when the spacecraft were well situated to acquire detailed observations in the plasma sheet. These data are compared to ground-based observations of Pi1B signatures in order to characterize differences in onset times and to determine the extent to which these observations are correlated.

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